Probing dark energy with future redshift surveys: A comparison of emission line and broad band selection in the near infrared

Details Probing dark energy with future redshift surveys: A comparison of emission line and broad band selection in the near infrared Probing dark energy with future redshift surveys: A comparison of emission line and broad band selection in the near infrared

2009-11-03

arxiv.org/abs/0911.0669v1

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

submitted to MNRAS

Scientific paper

Future galaxy surveys will map the galaxy distribution in the redshift interval $0.5 -15.4$; a flux limit of at least $\logfha = -16$ is required for an \ha sample to become competitive in effective volume.

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